Red Dwarfs: Their Geological, Chemical, and Biological Potential for Life
Autor David S. Stevensonen Limba Engleză Hardback – 25 sep 2019
This thought-provoking book looks at the nature of red dwarf systems as potential homes for life. Realistically, what are the prospects for life on these distant worlds? Could life evolve and survive there? How do these planetary surfaces and geologies evolve? How would life on a planet orbiting a red dwarf differ from life on Earth? And what are the implications for finding further habitable worlds in our galaxy?
The author provides readers with insight into the habitability of planets and how this changes as time progresses and the central star evolves. Since the previous 2013 edition Under a Crimson Sun, there has been a rise in newly discovered planets orbiting red dwarfs, accompanied by controversial areas of research that test what we think we know about these systems. This revised edition delves into the wealth of new material uncovered since that date. It explains the often conflicting results and analyses put forward and clarifies our understanding of these exciting new worlds.
The chapters explore the full width of relevant scientific discovery and speculation on the potential for red dwarf planets to host life. New content includes improved atmospheric models, new understandings of the impact of stellar radiation on the atmosphere of red dwarf worlds, tidal-locking, and comparisons with terrestrial geology and climate.The author provides readers with insight into the habitability of planets and how this changes as time progresses and the central star evolves. Since the previous 2013 edition Under a Crimson Sun, there has been a rise in newly discovered planets orbiting red dwarfs, accompanied by controversial areas of research that test what we think we know about these systems. This revised edition delves into the wealth of new material uncovered since that date. It explains the often conflicting results and analyses put forward and clarifies our understanding of these exciting new worlds.
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Specificații
ISBN-13: 9783030255497
ISBN-10: 3030255492
Pagini: 370
Ilustrații: XIII, 370 p. 114 illus. in color.
Dimensiuni: 155 x 235 mm
Greutate: 0.72 kg
Ediția:2nd ed. 2019
Editura: Springer International Publishing
Colecția Springer
Locul publicării:Cham, Switzerland
ISBN-10: 3030255492
Pagini: 370
Ilustrații: XIII, 370 p. 114 illus. in color.
Dimensiuni: 155 x 235 mm
Greutate: 0.72 kg
Ediția:2nd ed. 2019
Editura: Springer International Publishing
Colecția Springer
Locul publicării:Cham, Switzerland
Cuprins
Preface.- Chapter 1: The Formation of Stars and Planets at the Bottom of the Main Sequence.- Chapter 2: Exoplanetary Discovery.- Chapter 3: Planetary Tectonism.- Chapter 4: Deep Cycles and Super-Terrans.- Chapter 5: Atmospheric Circulation and Climate.- Chapter 6: The Origin and Early Evolution of Life.- Chapter 7: The Niche, Its Hypervolume and the Entropy of Existence.- Chapter 8: The Failure of Early Optimism.- Chapter 9: A New Hope.- Glossary.- Index.
Notă biografică
David Stevenson was born in Paisley, Scotland, in 1968. He studied Molecular Biology at Glasgow University and obtained a PhD in Genetics from the University of Cambridge. He then studied Astronomy and Planetary Sciences and Geophysics and Geochemistry (S267) at the OU.
After a stint in academia, Stevenson became a teacher, but continued to write science articles for various publications. In July 2007 an article on Type Ia Supernovae, “A Bigger Bang,” was published in Sky & Telescope, with a second article on supernovae published in the same magazine in October 2011. Three books have followed on supernovae, red dwarf stars and star clusters (Extreme Explosions, Under a Crimson Sun and The Complex Life of Star Clusters, respectively). A further article on stellar mergers is at the production stages with Astronomy magazine, while a spin-off article from Extreme Explosions, “Supersized Stellar Mystery,” was published in Popular Astronomyin February 2014.
Despite a background in Biology, the author’s father inspired his interest in Astronomy from an early age. Many parallels can be drawn between the lives of people and those of stars -- a thought that is explored in his most recent Springer book, The Nature of Life and Its Potential to Survive. Exploring the cross-roads of different scientific disciplines is a key interest and motivation in both Stevenson's teaching and writing.
After a stint in academia, Stevenson became a teacher, but continued to write science articles for various publications. In July 2007 an article on Type Ia Supernovae, “A Bigger Bang,” was published in Sky & Telescope, with a second article on supernovae published in the same magazine in October 2011. Three books have followed on supernovae, red dwarf stars and star clusters (Extreme Explosions, Under a Crimson Sun and The Complex Life of Star Clusters, respectively). A further article on stellar mergers is at the production stages with Astronomy magazine, while a spin-off article from Extreme Explosions, “Supersized Stellar Mystery,” was published in Popular Astronomyin February 2014.
Despite a background in Biology, the author’s father inspired his interest in Astronomy from an early age. Many parallels can be drawn between the lives of people and those of stars -- a thought that is explored in his most recent Springer book, The Nature of Life and Its Potential to Survive. Exploring the cross-roads of different scientific disciplines is a key interest and motivation in both Stevenson's teaching and writing.
Textul de pe ultima copertă
This thought-provoking book looks at the nature of red dwarf systems as potential homes for life. Realistically, what are the prospects for life on these distant worlds? Could life evolve and survive there? How do these planetary surfaces and geologies evolve? How would life on a planet orbiting a red dwarf differ from life on Earth? And what are the implications for finding further habitable worlds in our galaxy?
The author provides readers with insight into the habitability of planets and how this changes as time progresses and the central star evolves. Since the previous 2013 edition Under a Crimson Sun, there has been a rise in newly discovered planets orbiting red dwarfs, accompanied by controversial areas of research that test what we think we know about these systems. This revised edition delves into the wealth of new material uncovered since that date. It explains the often conflicting results and analyses put forward and clarifies our understanding of these exciting new worlds.
The chapters explore the full width of relevant scientific discovery and speculation on the potential for red dwarf planets to host life. New content includes improved atmospheric models, new understandings of the impact of stellar radiation on the atmosphere of red dwarf worlds, tidal-locking, and comparisons with terrestrial geology and climate.The author provides readers with insight into the habitability of planets and how this changes as time progresses and the central star evolves. Since the previous 2013 edition Under a Crimson Sun, there has been a rise in newly discovered planets orbiting red dwarfs, accompanied by controversial areas of research that test what we think we know about these systems. This revised edition delves into the wealth of new material uncovered since that date. It explains the often conflicting results and analyses put forward and clarifies our understanding of these exciting new worlds.
Caracteristici
Combines knowledge from various fields in a cohesive multidisciplinary approach Written in an accessible and reader-friendly style Contains a plethora of chapter references and suggestions for further reading